Dynamic Time Lag Regression: Predicting What & When

Authors: Mandar Chandorkar, Cyril Furtlehner, Bala Poduval, Enrico Camporeale, Michele Sebag

ICLR 2020 | Conference PDF | Archive PDF | Plain Text | LLM Run Details

Reproducibility Variable Result LLM Response
Research Type Experimental A proof of concept on synthetic problems is presented. Finally, the empirical results on the solar wind modelling task improve on the state of the art in solar wind forecasting.
Researcher Affiliation Academia Mandar Chandorkar Centrum Wiskunde en Informatica Amsterdam 1098XG Cyril Furtlehner INRIA-Saclay Bala Poduval University of New Hampshire Durham, NH 03824 Enrico Camporeale CIRES, University of Colorado Boulder, CO Michèle Sebag CNRS Univ. Paris-Saclay
Pseudocode Yes Algorithm 1: DTLR algorithm
Open Source Code No The algorithm code is available in supplementary material and will be made public after the reviewing period.
Open Datasets Yes The cause series xt includes the solar magnetic ... produced by the Current Sheet Source Surface model (Zhao and Hoeksema, 1995; Poduval and Zhao, 2014; Poduval, 2016)... The effect series, the hourly solar wind data is available from the OMNI data base from the Space Physics Data Facility 5. Footnote 5 provides the URL https://omniweb.gsfc.nasa.gov.
Dataset Splits Yes DTLR is validated using a nine fold cross-validation (Table 3 in appendix), where each fold is a continuous period corresponding to a solar rotation.
Hardware Specification No The paper does not specify any hardware details such as CPU or GPU models used for experiments.
Software Dependencies No The paper mentions neural network architectures and activation functions (Re Lu, Sigmoid) but does not provide specific version numbers for any software libraries or frameworks used.
Experiment Setup Yes The initialization of hyper-parameters α and σ is settled using preliminary experiments (same setting for all considered problems: α U(0.75, 2); σ2 U(10 5, 5))." and "Table 4: Network Architecture Details ... Layer sizes Activations ... I 2 [40, 40] [Re LU, Sigmoid]